A Case Study of Low-Mass Star Formation
Astrophysics
2019-08-19 v1
Abstract
This article synthesizes observational data from an extensive program aimed toward a comprehensive understanding of star formation in a low-mass star-forming molecular cloud. New observations and published data spanning from the centimeter wave band to the near infrared reveal the high and low density molecular gas, dust, and pre-main sequence stars in L1551.
Cite
@article{arxiv.0706.2206,
title = {A Case Study of Low-Mass Star Formation},
author = {J. Swift and Wm. J. Welch},
journal= {arXiv preprint arXiv:0706.2206},
year = {2019}
}